An andesitic source for Jack Hills zircon supports onset of plate tectonics in the Hadean

© 2020 Crown. The composition and origin of Earth’s early crust remains hotly debated. Here we use partition coefficients to invert the trace element composition of 4.3–3.3 Gyr Jack Hills zircons to calculate the composition of the melts from which they crystallised. Using this approach, the ave...

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Main Authors: Turner, S., Wilde, Simon, Wörner, G., Schaefer, B., Lai, Y.J.
Format: Journal Article
Language:English
Published: 2020
Online Access:http://hdl.handle.net/20.500.11937/81785
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author Turner, S.
Wilde, Simon
Wörner, G.
Schaefer, B.
Lai, Y.J.
author_facet Turner, S.
Wilde, Simon
Wörner, G.
Schaefer, B.
Lai, Y.J.
author_sort Turner, S.
building Curtin Institutional Repository
collection Online Access
description © 2020 Crown. The composition and origin of Earth’s early crust remains hotly debated. Here we use partition coefficients to invert the trace element composition of 4.3–3.3 Gyr Jack Hills zircons to calculate the composition of the melts from which they crystallised. Using this approach, the average SiO2 content of these melts was 59 ± 6 wt. % with Th/Nb, Dy/Yb and Sr/Y ratios of 2.7 ± 1.9, 0.9 ± 0.2 and 1.6 ± 0.7, respectively. Such features strongly indicate that the protolith for the Jack Hills zircons was not an intra-plate mafic rock, nor a TTG (tondjhemite-tonalite-granodiorite) or a Sudbury-like impact melt. Instead, the inferred equilibrium melts are much more similar to andesites formed in modern subduction settings. We find no evidence for any secular variation between 4.3 and 3.3 Gyr implying little change in the composition or tectonic affinity of the Earth’s early crust from the Hadean to Mesoarchaean.
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spelling curtin-20.500.11937-817852020-12-15T04:26:47Z An andesitic source for Jack Hills zircon supports onset of plate tectonics in the Hadean Turner, S. Wilde, Simon Wörner, G. Schaefer, B. Lai, Y.J. © 2020 Crown. The composition and origin of Earth’s early crust remains hotly debated. Here we use partition coefficients to invert the trace element composition of 4.3–3.3 Gyr Jack Hills zircons to calculate the composition of the melts from which they crystallised. Using this approach, the average SiO2 content of these melts was 59 ± 6 wt. % with Th/Nb, Dy/Yb and Sr/Y ratios of 2.7 ± 1.9, 0.9 ± 0.2 and 1.6 ± 0.7, respectively. Such features strongly indicate that the protolith for the Jack Hills zircons was not an intra-plate mafic rock, nor a TTG (tondjhemite-tonalite-granodiorite) or a Sudbury-like impact melt. Instead, the inferred equilibrium melts are much more similar to andesites formed in modern subduction settings. We find no evidence for any secular variation between 4.3 and 3.3 Gyr implying little change in the composition or tectonic affinity of the Earth’s early crust from the Hadean to Mesoarchaean. 2020 Journal Article http://hdl.handle.net/20.500.11937/81785 10.1038/s41467-020-14857-1 eng http://creativecommons.org/licenses/by/4.0/ fulltext
spellingShingle Turner, S.
Wilde, Simon
Wörner, G.
Schaefer, B.
Lai, Y.J.
An andesitic source for Jack Hills zircon supports onset of plate tectonics in the Hadean
title An andesitic source for Jack Hills zircon supports onset of plate tectonics in the Hadean
title_full An andesitic source for Jack Hills zircon supports onset of plate tectonics in the Hadean
title_fullStr An andesitic source for Jack Hills zircon supports onset of plate tectonics in the Hadean
title_full_unstemmed An andesitic source for Jack Hills zircon supports onset of plate tectonics in the Hadean
title_short An andesitic source for Jack Hills zircon supports onset of plate tectonics in the Hadean
title_sort andesitic source for jack hills zircon supports onset of plate tectonics in the hadean
url http://hdl.handle.net/20.500.11937/81785